1 Ocak 2016 Dergi makalesi Açık Erişim

Khachatryan, V.; Sirunyan, A. M.; Tumasyan, A.; Adam, W.; Asilar, E.; Bergauer, T.; Brandstetter, J.; Brondolin, E.; Dragicevic, M.; Eroe, J.; Flechl, M.; Friedl, M.; Fruehwirth, R.; Ghete, V. M.; Hartl, C.; Hoermann, N.; Hrubec, J.; Jeitler, M.; Knuenz, V.; Koenig, A.; Koenig, A.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/54223</identifier>
  <creators>
    <creator>
      <creatorName>Khachatryan, V.</creatorName>
      <givenName>V.</givenName>
      <familyName>Khachatryan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation>
    </creator>
    <creator>
      <creatorName>Sirunyan, A. M.</creatorName>
      <givenName>A. M.</givenName>
      <familyName>Sirunyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation>
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      <creatorName>Tumasyan, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Tumasyan</familyName>
      <affiliation>Yerevan Phys Inst, Yerevan 375036, Armenia</affiliation>
    </creator>
    <creator>
      <creatorName>Adam, W.</creatorName>
      <givenName>W.</givenName>
      <familyName>Adam</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Asilar, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Asilar</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Bergauer, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Bergauer</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Brandstetter, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Brandstetter</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Brondolin, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Brondolin</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Dragicevic, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Dragicevic</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Eroe, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Eroe</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Flechl, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Flechl</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Friedl, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Friedl</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Fruehwirth, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Fruehwirth</familyName>
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    <creator>
      <creatorName>Ghete, V. M.</creatorName>
      <givenName>V. M.</givenName>
      <familyName>Ghete</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Hartl, C.</creatorName>
      <givenName>C.</givenName>
      <familyName>Hartl</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Hoermann, N.</creatorName>
      <givenName>N.</givenName>
      <familyName>Hoermann</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Hrubec, J.</creatorName>
      <givenName>J.</givenName>
      <familyName>Hrubec</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Jeitler, M.</creatorName>
      <givenName>M.</givenName>
      <familyName>Jeitler</familyName>
    </creator>
    <creator>
      <creatorName>Knuenz, V.</creatorName>
      <givenName>V.</givenName>
      <familyName>Knuenz</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Koenig, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Koenig</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
    <creator>
      <creatorName>Koenig, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Koenig</familyName>
      <affiliation>OeAW, Inst Hochenergiephys, Vienna, Austria</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Search For Narrow Resonances Decaying To Dijets In Proton-Proton Collisions At Root S=13 Tev</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2016</publicationYear>
  <dates>
    <date dateType="Issued">2016-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/54223</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/PhysRevLett.116.071801</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">A search for narrow resonances in proton-proton collisions at root s = 13 TeV is presented. The invariant mass distribution of the two leading jets is measured with the CMS detector using a data set corresponding to an integrated luminosity of 2.4 fb(-1). The highest observed dijet mass is 6.1 TeV. The distribution is smooth and no evidence for resonant particles is observed. Upper limits at 95% confidence level are set on the production cross section for narrow resonances with masses above 1.5 TeV. When interpreted in the context of specific models, the limits exclude string resonances with masses below 7.0 TeV, scalar diquarks below 6.0 TeV, axigluons and colorons below 5.1 TeV, excited quarks below 5.0 TeV, color-octet scalars below 3.1 TeV, and W' bosons below 2.6 TeV. These results significantly extend previously published limits.</description>
  </descriptions>
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